The formation of the Milky Way halo and its dwarf satellites; a NLTE-1D abundance analysis II. Early chemical enrichment (vol 608, A89, 2017)

被引:1
作者
Mashonkina, L. [1 ,2 ]
Jablonka, P. [3 ,4 ]
Sitnova, T. [2 ]
Pakhomov, Yu. [2 ]
North, P. [3 ]
机构
[1] Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany
[2] Russian Acad Sci, Inst Astron, Moscow 119017, Russia
[3] Ecole Polytech Fed Lausanne EPFL, Observ Sauverny, Lab Astrophys, CH-1290 Versoix, Switzerland
[4] Univ Paris Diderot, CNRS, Observ Paris, GEPI, F-92125 Meudon, France
关键词
line: formation; nuclear reactions; nucleosynthesis; abundances; stars: abundances; stars: atmospheres; galaxies: abundances; errata; addenda;
D O I
10.1051/0004-6361/201731582e
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页数:2
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[1]   The formation of the Milky Way halo and its dwarf satellites; a NLTE-1D abundance analysis II. Early chemical enrichment [J].
Mashonkina, L. ;
Jablonka, P. ;
Sitnova, T. ;
Pakhomov, Yu. ;
North, P. .
ASTRONOMY & ASTROPHYSICS, 2017, 608